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Final Project - The Astroid

by

Lydia Silva and Brianne Yokoyama

What is an Astroid?

According to Wolfram MathWorld’s website, an astroid is “A 4-cusped hypocycloid which is sometimes also called a tetracuspid, cubocycloid, or paracycle.” To clearly understand this definition, it is necessary to explain a few of these geometric terms more fully.

A hypocycloid is the curve traced by a point on a circle of radius r which is being rolled along the inside circumference of another circle of a larger radius R

A cusp is defined to be a “point at which two branches of a curve meet such that the tangents of each branch are equal.”

An astroid is a specialized case of the general hypocycloid family of curves. When you have two circles, one with a radius of R, and the other with a radius of r, where r is ¼ the length of R, the resulting curve is a star-like shape with four points or cusps. This curve was given the simple name astroid in 1836. The word astroid is the term from which the modern word asteroid is derived.

The relation between the number of cusps and the ratio of lengths R to r is simple. The formation of a cusp occurs every time the smaller circle completes a full rotation along the inside of the larger circle. To roll all the way around the inside of the larger circle, it must make R/r rotations. In the case of the astroid, the smaller circle which we will call circle 1 has a circumference that is precisely ¼ that of the larger circle, circle 2. Therefore, as circle 1 is rolled along the inside of the circle 2, it must make four revolutions before returning to its original position, resulting in a curve with four cusps.

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The equation for the astroid in Cartesian coordinates is x2/3+y2/3=a2/3

For a simple parametrization of the curve you can substitute u for x1/3 and v for y1/3 and r for a1/3  and the equation becomes u2 +v2=r2. Using the parameters u=rcos(t) and v=rsin(t) and substituting our x,y, and z values, we get the following parametric equations:

x1/3= a1/3 cos(t)

(x1/3)3=( a1/3 cos(t))3

x=acos3(t)

 

y1/3= a1/3 sin(t)

(y1/3)3=( a1/3 sin(t))3

y=asin3(t)

 



The Danish astronomer Ole Roemer, famed for his discovery that light has a finite velocity, first discovered the astroid curve in 1674 in studying applications of the properties of hypocycloids in relation to gear teeth. Scientists and mathematicians Johann Bernoulli, Gottfried Leibniz, and Jean Le Rond d’Alembert performed further investigations of the astroid. In 1725, David Bernoulli discovered the double generation property of the astroid. His work showed that the astroid curved traced within a circle of radius R is created by two circles, not just one. The first we already know has a radius of ¼R, but the second will have a radius of ¾R.

 

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You can use astroids to make many interesting patterns such as the Astroid Diamond shown below.

 

 

References:

Lee, Xha. “Astroid”, Visual Dictionary of Specialized Curves, 2004, 13 May, 2007 http://xahlee.org/SpecialPlaneCurves_dir/Astroid_dir/astroid.html

“Ole Roemer” Love to Know Website, 29 Aug. 2007. 13 May 2007 <http://www.1911encyclopedia.org/Ole_Roemer>

Wassenar, Jan. “Astroid”, Mathematical Curves, Roullette. 13 March 2005. 13 May 2007http://www.2dcurves.com/roulette/roulettea.html

Weisstein, Eric W. "Astroid." From MathWorld--A Wolfram Web Resource. http://mathworld.wolfram.com/Astroid.html

O’Hanen, Benjamin and Matthew Wisan. “The Asteroids: Special Planes Curve.” 15 May 2006. 13 May 2007 <http://online.redwoods.cc.ca.us/instruct/darnold/CalcProj/sp06/mattben/RealWebsite/AsteroidPaper.html>